The topology of magnetic reconnection in solar flares
In order to better understand the location and evolution of magnetic reconnection, which is thought to be the energy release mechanism in solar flares, I combine the analysis of hard X-ray (HXR) sources observed by RHESSI with a three-dimensional, quantitative magnetic charge topology (MCT) model. I...
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| Language: | en |
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2007
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| Online Access: | http://etd.lib.montana.edu/etd/2007/desjardins/DesJardinsA0807.pdf |